D. H. Beck
University of Illinois at Urbana-Champaign
H-index: 195
North America-United States
About D. H. Beck
D. H. Beck, With an exceptional h-index of 195 and a recent h-index of 142 (since 2020), a distinguished researcher at University of Illinois at Urbana-Champaign,
His recent articles reflect a diverse array of research interests and contributions to the field:
1: 2 AV CONDUCTION LEADING TO INAPPROPRIATE ICD SHOCK
NSR Query Results
Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
A Natural Field-like Entanglement Resource in Trapped-Ion Chains
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers
Entanglement structures in quantum field theories. II. Distortions of vacuum correlations through the lens of local observers
BICEP/Keck. XVI. Characterizing dust polarization through correlations with neutral hydrogen
D. H. Beck Information
University | University of Illinois at Urbana-Champaign |
|---|---|
Position | Professor of Physics |
Citations(all) | 166605 |
Citations(since 2020) | 85133 |
Cited By | 83612 |
hIndex(all) | 195 |
hIndex(since 2020) | 142 |
i10Index(all) | 944 |
i10Index(since 2020) | 785 |
University Profile Page | University of Illinois at Urbana-Champaign |
Top articles of D. H. Beck
1: 2 AV CONDUCTION LEADING TO INAPPROPRIATE ICD SHOCK
Authors
Iain J Thompson,David Gittess,Hiroko Beck,William M Miles,Steven J Ross
Journal
Journal of the American College of Cardiology
Published Date
2024/4/2
BackgroundDual AV nodal physiology describes the ability of the AV node (AVN) to conduct using two distinct pathways, a fast AV nodal pathway and a slow pathway. Most commonly this results in AVNRT. Rarely, it can allow for a phenomenon known as 1: 2 AV conduction. 1: 2 AV conduction denotes one atrial impulse giving way to two ventricular depolarizations. This is often incorrectly interpreted as a tachyarrhythmia. Herein, we report a case of 1: 2 AV condition resulting in erroneous ICD recognition of VT and inappropriate ICD therapies.
NSR Query Results
Authors
PE Garrett,TR Rodriguez,A Diaz Varela,KL Green,J Bangay,A Finlay,RAE Austin,GC Ball,DS Bandyopadhyay,V Bildstein,S Colosimo,DS Cross,GA Demand,P Finlay,AB Garnsworthy,GF Grinyer,G Hackman,B Jigmeddorj,J Jolie,WD Kulp,KG Leach,AC Morton,JN Orce,CJ Pearson,AA Phillips,AJ Radich,ET Rand,MA Schumaker,CE Svensson,C Sumithrarachchi,S Triambak,N Warr,J Wong,JL Wood,SW Yates
Journal
Phys. Rev. C
Published Date
2020
NUCLEAR REACTIONS 3 He (32 S, α) 31 S, E= 128 MeV; measured reaction products, Eγ, Iγ; deduced γ-ray energies, levels, T 1/2, resonances. Comparison with the shell-model code NuShellX calculations. Modern Markov chain Monte Carlo-based Bayesian statistical techniques. The Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility.
Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
Authors
Unni Fuskeland,J Aumont,R Aurlien,C Baccigalupi,AJ Banday,HK Eriksen,J Errard,RT Génova-Santos,T Hasebe,J Hubmayr,H Imada,N Krachmalnicoff,L Lamagna,G Pisano,D Poletti,M Remazeilles,KL Thompson,L Vacher,Ingunn Kathrine Wehus,S Azzoni,M Ballardini,RB Barreiro,N Bartolo,Artem Basyrov,D Beck,M Bersanelli,M Bortolami,Maksym Brilenkov,E Calabrese,A Carones,FJ Casas,K Cheung,J Chluba,SE Clark,L Clermont,F Columbro,A Coppolecchia,G D’Alessandro,P De Bernardis,T De Haan,E De La Hoz,M De Petris,S Della Torre,P Diego-Palazuelos,F Finelli,C Franceschet,G Galloni,Mathew Galloway,M Gerbino,M Gervasi,T Ghigna,S Giardiello,Eirik Gjerløw,A Gruppuso,P Hargrave,M Hattori,M Hazumi,LT Hergt,D Herman,D Herranz,E Hivon,TD Hoang,K Kohri,M Lattanzi,AT Lee,C Leloup,F Levrier,AI Lonappan,G Luzzi,B Maffei,E Martínez-González,S Masi,S Matarrese,T Matsumura,M Migliaccio,L Montier,G Morgante,B Mot,L Mousset,R Nagata,T Namikawa,F Nati,P Natoli,S Nerval,A Novelli,L Pagano,A Paiella,D Paoletti,G Pascual-Cisneros,G Patanchon,V Pelgrims,F Piacentini,G Piccirilli,G Polenta,G Puglisi,N Raffuzzi,A Ritacco,JA Rubino-Martin,G Savini,D Scott,Y Sekimoto,M Shiraishi,G Signorelli,SL Stever,N Stutzer,RM Sullivan,H Takakura,L Terenzi,Harald Thommesen,M Tristram,M Tsuji,P Vielva,J Weller,B Westbrook,G Weymann-Despres,EJ Wollack,M Zannoni
Journal
Astronomy & Astrophysics
Published Date
2023/8/1
LiteBIRD is a planned JAXA-led cosmic microwave background (CMB) B-mode satellite experiment aiming for launch in the late 2020s, with a primary goal of detecting the imprint of primordial inflationary gravitational waves. Its current baseline focal-plane configuration includes 15 frequency bands between 40 and 402 GHz, fulfilling the mission requirements to detect the amplitude of gravitational waves with the total uncertainty on the tensor-to-scalar ratio, δr, down to δr < 0.001. A key aspect of this performance is accurate astrophysical component separation, and the ability to remove polarized thermal dust emission is particularly important. In this paper we note that the CMB frequency spectrum falls off nearly exponentially above 300 GHz relative to the thermal dust spectral energy distribution, and a relatively minor high frequency extension can therefore result in even lower uncertainties and better model …
A Natural Field-like Entanglement Resource in Trapped-Ion Chains
Authors
Natalie Klco,DH Beck
Journal
arXiv preprint arXiv:2311.08842
Published Date
2023/11/15
The electromagnetic trapping of ion chains can be regarded as a process of non-trivial entangled quantum state preparation within Hilbert spaces of the local axial motional modes. To begin uncovering properties of this entanglement resource produced as a byproduct of conventional ion-trap quantum information processing, the quantum continuous-variable formalism is herein utilized to focus on the leading-order entangled ground state of local motional modes in the presence of a quadratic trapping potential. The decay of entanglement between disjoint subsets of local modes is found to exhibit features of entanglement structure and response to partial measurement reminiscent of the free massless scalar field vacuum. With significant fidelities between the two, even for large system sizes, a framework is established for initializing quantum field simulations via "imaging" extended entangled states from natural sources, rather than building correlations through deep circuits of few-body entangling operators. By calculating probabilities in discrete Fock subspaces of the local motional modes, considerations are presented for locally transferring these pre-distributed entanglement resources to the qudits of ion internal energy levels, improving this procedure's anticipated experimental viability.
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
Authors
LiteBIRD Collaboration,E Allys,K Arnold,J Aumont,R Aurlien,S Azzoni,C Baccigalupi,AJ Banday,R Banerji,RB Barreiro,N Bartolo,L Bautista,D Beck,S Beckman,M Bersanelli,F Boulanger,M Brilenkov,M Bucher,E Calabrese,P Campeti,A Carones,FJ Casas,A Catalano,V Chan,K Cheung,Y Chinone,SE Clark,F Columbro,G D’Alessandro,P de Bernardis,T de Haan,E de la Hoz,M De Petris,S Della Torre,P Diego-Palazuelos,M Dobbs,T Dotani,JM Duval,T Elleflot,HK Eriksen,J Errard,T Essinger-Hileman,F Finelli,R Flauger,C Franceschet,U Fuskeland,M Galloway,K Ganga,M Gerbino,M Gervasi,RT Génova-Santos,T Ghigna,S Giardiello,E Gjerløw,J Grain,F Grupp,A Gruppuso,JE Gudmundsson,NW Halverson,P Hargrave,T Hasebe,M Hasegawa,M Hazumi,S Henrot-Versillé,B Hensley,LT Hergt,D Herman,E Hivon,RA Hlozek,AL Hornsby,Y Hoshino,J Hubmayr,K Ichiki,T Iida,H Imada,H Ishino,G Jaehnig,N Katayama,A Kato,R Keskitalo,T Kisner,Y Kobayashi,A Kogut,K Kohri,E Komatsu,K Komatsu,K Konishi,N Krachmalnicoff,CL Kuo,L Lamagna,M Lattanzi,AT Lee,C Leloup,F Levrier,E Linder,G Luzzi,J Macias-Perez,T Maciaszek,B Maffei,D Maino,S Mandelli,E Martínez-González,S Masi,M Massa,S Matarrese,FT Matsuda,T Matsumura,L Mele,M Migliaccio,Y Minami,A Moggi,J Montgomery,L Montier,G Morgante,B Mot,Y Nagano,T Nagasaki,R Nagata,R Nakano,T Namikawa,F Nati,P Natoli,S Nerval,F Noviello,K Odagiri,S Oguri,H Ohsaki,L Pagano,A Paiella,D Paoletti,A Passerini,G Patanchon,F Piacentini,M Piat,G Pisano,G Polenta,D Poletti,T Prouvé,G Puglisi,D Rambaud,C Raum,S Realini,M Reinecke,M Remazeilles,A Ritacco,G Roudil,JA Rubino-Martin,M Russell,H Sakurai,Y Sakurai
Published Date
2023/4
LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency (JAXA) selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with an expected launch in the late 2020s using JAXA’s H3 rocket. LiteBIRD is planned to orbit the Sun–Earth Lagrangian point L2, where it will map the cosmic microwave background polarization over the entire sky for three years, with three telescopes in 15 frequency bands between 34 and 448 GHz, to achieve an unprecedented total sensitivity of K-arcmin, with a typical angular resolution of 0.5○ at 100 GHz. The primary scientific objective of LiteBIRD is to search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models …
Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers
Authors
Sofia Fatigoni,Peter AR Ade,Z Ahmed,Mandana Amiri,Denis Barkats,R Basu Thakur,Colin A Bischoff,Dominic Beck,James J Bock,Victor Buza,J Cheshire,Jake Connors,James Cornelison,Michael Crumrine,Ari Josef Cukierman,EV Denison,MI Dierickx,Lionel Duband,M Eiben,Jeff P Filippini,C Giannakopoulos,N Goeckner-Wald,DC Goldfinger,JA Grayson,PK Grimes,G Hall,G Halal,M Halpern,E Hand,SA Harrison,S Handerson,SR Hildebrandt,GC Hilton,J Hubmayr,H Hui,KD Irwin,J Kang,KS Karkare,S Kefeli,JM Kovac,CL Kuo,K Lau,EM Leitch,A Lennox,T Liu,KG Megerian,OY Miller,L Minutolo,L Moncelsi,Y Nakato,T Namikawa,Hien T Nguyen,RO Brient,Steven Palladino,Matthew A Petroff,N Namikawa,Thomas Prouve,Clement Pryke,Benjamin Racine,Carl D Reintsema,Thibault Romand,Maria Salatino,Alessandro Schillaci,BL Schmitt,Baibhav Singari,Ahmed Soliman,T St Germaine,Aaron Steiger,Bryan Steinbach,RV Sudiwala,Keith L Thompson,C Tucker,AD Turner,C Umilta,C Verges,AG Vieregg,Albert Wandui,Alexis C Weber,DV Wiebe,Justin Willmert,Wai Ling K Wu,E Yang,KW Yoon,E Young,C Yu,L Zeng,C Zhang,S Zhang
Journal
arXiv preprint arXiv:2310.10849
Published Date
2023/10/16
Time-Division Multiplexing is the readout architecture of choice for many ground and space experiments, as it is a very mature technology with proven outstanding low-frequency noise stability, which represents a central challenge in multiplexing. Once fully populated, each of the two BICEP Array high frequency receivers, observing at 150GHz and 220/270GHz, will have 7776 TES detectors tiled on the focal plane. The constraints set by these two receivers required a redesign of the warm readout electronics. The new version of the standard Multi Channel Electronics, developed and built at the University of British Columbia, is presented here for the first time. BICEP Array operates Time Division Multiplexing readout technology to the limits of its capabilities in terms of multiplexing rate, noise and crosstalk, and applies them in rigorously demanding scientific application requiring extreme noise performance and systematic error control. Future experiments like CMB-S4 plan to use TES bolometers with Time Division/SQUID-based readout for an even larger number of detectors.
Entanglement structures in quantum field theories. II. Distortions of vacuum correlations through the lens of local observers
Authors
Natalie Klco,DH Beck
Journal
Physical Review A
Published Date
2023/7/24
When observing a quantum field via detectors with access to only the mixed states of spatially separated, local regions—a ubiquitous experimental design—the capacity to access the full extent of distributed entanglement can be limited, shrouded by classical correlations. By performing projective measurements of the field external to two detection patches and classically communicating the results, underlying pure states may be identified for which entanglement quantification is clear. In the Gaussian continuous-variable states of the free scalar field vacuum, this protocol uncovers a disparity between the spacelike entanglement established within the field and that which is locally detectable. This discrepancy is found to grow exponentially with the separation between observation regions. The protocol developed herein offers insight and practical guidance for clarifying the unavoidable distortion of quantum field …
BICEP/Keck. XVI. Characterizing dust polarization through correlations with neutral hydrogen
Authors
PAR Ade,Z Ahmed,M Amiri,D Barkats,R Basu Thakur,CA Bischoff,D Beck,JJ Bock,H Boenish,E Bullock,V Buza,James R Cheshire,SE Clark,J Connors,J Cornelison,Mike Crumrine,A Cukierman,EV Denison,M Dierickx,L Duband,M Eiben,S Fatigoni,JP Filippini,Stefan Fliescher,C Giannakopoulos,N Goeckner-Wald,DC Goldfinger,J Grayson,P Grimes,G Hall,G Halal,M Halpern,E Hand,S Harrison,S Henderson,SR Hildebrandt,J Hubmayr,H Hui,KD Irwin,J Kang,KS Karkare,E Karpel,S Kefeli,SA Kernasovskiy,JM Kovac,CL Kuo,Kenny Lau,EM Leitch,A Lennox,KG Megerian,L Minutolo,L Moncelsi,Y Nakato,T Namikawa,HT Nguyen,R O’Brient,RW Ogburn IV,S Palladino,MA Petroff,T Prouve,C Pryke,B Racine,CD Reintsema,S Richter,A Schillaci,Robert Schwarz,BL Schmitt,CD Sheehy,B Singari,A Soliman,T St Germaine,B Steinbach,RV Sudiwala,GP Teply,KL Thompson,JE Tolan,C Tucker,AD Turner,C Umiltà,C Vergès,AG Vieregg,A Wandui,AC Weber,DV Wiebe,J Willmert,CL Wong,WLK Wu,H Yang,KW Yoon,E Young,C Yu,L Zeng,C Zhang,S Zhang,BICEP/Keck Collaboration
Journal
The Astrophysical Journal
Published Date
2023/3/8
We characterize Galactic dust filaments by correlating BICEP/Keck and Planck data with polarization templates based on neutral hydrogen (H i) observations. Dust polarization is important for both our understanding of astrophysical processes in the interstellar medium (ISM) and the search for primordial gravitational waves in the cosmic microwave background (CMB). In the diffuse ISM, H i is strongly correlated with the dust and partly organized into filaments that are aligned with the local magnetic field. We analyze the deep BICEP/Keck data at 95, 150, and 220 GHz, over the low-column-density region of sky where BICEP/Keck has set the best limits on primordial gravitational waves. We separate the H i emission into distinct velocity components and detect dust polarization correlated with the local Galactic H i but not with the H i associated with Magellanic Stream i. We present a robust, multifrequency detection of …
Search for two-neutrino double-beta decay of 136Xe to the excited state of 136Ba with the complete EXO-200 dataset
Authors
S Al Kharusi,G Anton,I Badhrees,PS Barbeau,D Beck,V Belov,T Bhatta,M Breidenbach,T Brunner,GF Cao,WR Cen,C Chambers,B Cleveland,M Coon,A Craycraft,T Daniels,L Darroch,SJ Daugherty,J Davis,S Delaquis,A Der Mesrobian-Kabakian,R DeVoe,J Dilling,A Dolgolenko,MJ Dolinski,J Echevers,W Fairbank Jr,D Fairbank,J Farine,S Feyzbakhsh,P Fierlinger,YS Fu,D Fudenberg,P Gautam,R Gornea,G Gratta,C Hall,EV Hansen,J Hoessl,P Hufschmidt,M Hughes,A Iverson,A Jamil,C Jessiman,MJ Jewell,A Johnson,A Karelin,LJ Kaufman,T Koffas,R Krücken,A Kuchenkov,KS Kumar,Y Lan,A Larson,BG Lenardo,DS Leonard,GS Li,S Li,Z Li,C Licciardi,YH Lin,R MacLellan,T McElroy,T Michel,B Mong,DC Moore,K Murray,O Njoya,O Nusair,A Odian,I Ostrovskiy,A Perna,A Piepke,A Pocar,F Retière,AL Robinson,PC Rowson,J Runge,S Schmidt,D Sinclair,K Skarpaas,AK Soma,V Stekhanov,M Tarka,S Thibado,J Todd,T Tolba,TI Totev,R Tsang,B Veenstra,V Veeraraghavan,P Vogel,J-L Vuilleumier,M Wagenpfeil,J Watkins,M Weber,LJ Wen,U Wichoski,G Wrede,SX Wu,Q Xia,DR Yahne,L Yang,Y-R Yen,O Ya Zeldovich,T Ziegler,EXO-200 Collaboration
Journal
Chinese Physics C
Published Date
2023/10/1
A new search for two-neutrino double-beta (2νββ) decay of 136 Xe to the excited state of 136 Ba is performed with the full EXO-200 dataset. A deep learning-based convolutional neural network is used to discriminate signal from background events. Signal detection efficiency is increased relative to previous searches by EXO-200 by more than a factor of two. With the addition of the Phase II dataset taken with an upgraded detector, the median 90% confidence level half-life sensitivity of 2νββ decay to the state of 136 Ba is yr using a total 136 Xe exposure of 234.1 kg yr. No statistically significant evidence for 2νββ decay to the state is observed, leading to a lower limit of yr at 90% confidence level, improved by 70% relative to the current world's best constraint.
Generative adversarial networks for scintillation signal simulation in EXO-200
Authors
S Li,I Ostrovskiy,Z Li,Liang Yang,S Al Kharusi,G Anton,PS Barbeau,I Badhrees,D Beck,V Belov,T Bhatta,M Breidenbach,T Brunner,GF Cao,WR Cen,C Chambers,B Cleveland,M Coon,A Craycraft,T Daniels,L Darroch,SJ Daugherty,J Davis,S Delaquis,A Der Mesrobian-Kabakian,R DeVoe,J Dilling,A Dolgolenko,MJ Dolinski,J Echevers,W Fairbank,D Fairbank,J Farine,S Feyzbakhsh,P Fierlinger,YS Fu,D Fudenberg,P Gautam,R Gornea,G Gratta,C Hall,EV Hansen,J Hoessl,P Hufschmidt,M Hughes,A Iverson,A Jamil,C Jessiman,MJ Jewell,A Johnson,A Karelin,LJ Kaufman,T Koffas,R Krücken,A Kuchenkov,KS Kumar,Y Lan,A Larson,BG Lenardo,DS Leonard,GS Li,C Licciardi,YH Lin,R MacLellan,T McElroy,T Michel,B Mong,DC Moore,K Murray,O Njoya,O Nusair,A Odian,A Perna,A Piepke,A Pocar,F Retière,AL Robinson,PC Rowson,J Runge,S Schmidt,D Sinclair,K Skarpaas,AK Soma,V Stekhanov,M Tarka,S Thibado,J Todd,T Tolba,TI Totev,R Tsang,B Veenstra,V Veeraraghavan,P Vogel,J-L Vuilleumier,M Wagenpfeil,J Watkins,M Weber,LJ Wen,U Wichoski,G Wrede,SX Wu,Q Xia,DR Yahne,Y-R Yen,O Ya Zeldovich,T Ziegler
Journal
Journal of Instrumentation
Published Date
2023/6/5
Generative Adversarial Networks trained on samples of simulated or actual events have been proposed as a way of generating large simulated datasets at a reduced computational cost. In this work, a novel approach to perform the simulation of photodetector signals from the time projection chamber of the EXO-200 experiment is demonstrated. The method is based on a Wasserstein Generative Adversarial Network—a deep learning technique allowing for implicit non-parametric estimation of the population distribution for a given set of objects. Our network is trained on real calibration data using raw scintillation waveforms as input. We find that it is able to produce high-quality simulated waveforms an order of magnitude faster than the traditional simulation approach and, importantly, generalize from the training sample and discern salient high-level features of the data. In particular, the network correctly deduces …
LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
Authors
AI Lonappan,T Namikawa,G Piccirilli,P Diego-Palazuelos,M Ruiz-Granda,M Migliaccio,C Baccigalupi,N Bartolo,D Beck,K Benabed,A Challinor,J Errard,S Farrens,A Gruppuso,N Krachmalnicoff,E Martínez-González,V Pettorino,B Sherwin,J Starck,P Vielva,R Akizawa,A Anand,J Aumont,R Aurlien,S Azzoni,M Ballardini,AJ Banday,RB Barreiro,M Bersanelli,D Blinov,M Bortolami,T Brinckmann,E Calabrese,P Campeti,A Carones,F Carralot,FJ Casas,K Cheung,L Clermont,F Columbro,G Conenna,A Coppolecchia,F Cuttaia,G d'Alessandro,P de Bernardis,M De Petris,S Della Torre,E Di Giorgi,HK Eriksen,F Finelli,C Franceschet,U Fuskeland,G Galloni,M Galloway,M Georges,M Gerbino,M Gervasi,RT Génova-Santos,T Ghigna,S Giardiello,C Gimeno-Amo,E Gjerløw,M Hazumi,S Henrot-Versillé,LT Hergt,E Hivon,K Kohri,E Komatsu,L Lamagna,M Lattanzi,C Leloup,M Lembo,M López-Caniego,G Luzzi,J Macias-Perez,B Maffei,S Masi,M Massa,S Matarrese,T Matsumura,S Micheli,A Moggi,M Monelli,L Montier,G Morgante,B Mot,L Mousset,R Nagata,P Natoli,A Novelli,I Obata,A Occhiuzzi,L Pagano,A Paiella,D Paoletti,G Pascual-Cisneros,V Pavlidou,F Piacentini,M Pinchera,G Pisano,G Polenta,G Puglisi,M Remazeilles,A Ritacco,A Rizzieri,Y Sakurai,D Scott,M Shiraishi,G Signorelli,SL Stever,Y Takase,H Tanimura,A Tartari,K Tassis,L Terenzi,M Tristram,L Vacher,B van Tent,IK Wehus,G Weymann-Despres,M Zannoni,Y Zhou
Journal
arXiv preprint arXiv:2312.05184
Published Date
2023/12/8
We explore the capability of measuring lensing signals in $LiteBIRD$ full-sky polarization maps. With a $30$ arcmin beam width and an impressively low polarization noise of $2.16\,\mu$K-arcmin, $LiteBIRD$ will be able to measure the full-sky polarization of the cosmic microwave background (CMB) very precisely. This unique sensitivity also enables the reconstruction of a nearly full-sky lensing map using only polarization data, even considering its limited capability to capture small-scale CMB anisotropies. In this paper, we investigate the ability to construct a full-sky lensing measurement in the presence of Galactic foregrounds, finding that several possible biases from Galactic foregrounds should be negligible after component separation by harmonic-space internal linear combination. We find that the signal-to-noise ratio of the lensing is approximately $40$ using only polarization data measured over $90\%$ of the sky. This achievement is comparable to $Planck$'s recent lensing measurement with both temperature and polarization and represents a four-fold improvement over $Planck$'s polarization-only lensing measurement. The $LiteBIRD$ lensing map will complement the $Planck$ lensing map and provide several opportunities for cross-correlation science, especially in the northern hemisphere.
Quantum information science and technology for nuclear physics. Input into US Long-Range Planning, 2023
Authors
Douglas Beck,Joseph Carlson,Zohreh Davoudi,Joseph Formaggio,Sofia Quaglioni,Martin Savage,Joao Barata,Tanmoy Bhattacharya,Michael Bishof,Ian Cloet,Andrea Delgado,Michael DeMarco,Caleb Fink,Adrien Florio,Marianne Francois,Dorota Grabowska,Shannon Hoogerheide,Mengyao Huang,Kazuki Ikeda,Marc Illa,Kyungseon Joo,Dmitri Kharzeev,Karol Kowalski,Wai Kin Lai,Kyle Leach,Ben Loer,Ian Low,Joshua Martin,David Moore,Thomas Mehen,Niklas Mueller,James Mulligan,Pieter Mumm,Francesco Pederiva,Rob Pisarski,Mateusz Ploskon,Sanjay Reddy,Gautam Rupak,Hersh Singh,Maninder Singh,Ionel Stetcu,Jesse Stryker,Paul Szypryt,Semeon Valgushev,Brent VanDevender,Samuel Watkins,Christopher Wilson,Xiaojun Yao,Andrei Afanasev,Akif Baha Balantekin,Alessandro Baroni,Raymond Bunker,Bipasha Chakraborty,Ivan Chernyshev,Vincenzo Cirigliano,Benjamin Clark,Shashi Kumar Dhiman,Weijie Du,Dipangkar Dutta,Robert Edwards,Abraham Flores,Alfredo Galindo-Uribarri,Ronald Fernando Garcia Ruiz,Vesselin Gueorguiev,Fanqing Guo,Erin Hansen,Hector Hernandez,Koichi Hattori,Philipp Hauke,Morten Hjorth-Jensen,Keith Jankowski,Calvin Johnson,Denis Lacroix,Dean Lee,Huey-Wen Lin,Xiaohui Liu,Felipe J Llanes-Estrada,John Looney,Misha Lukin,Alexis Mercenne,Jeff Miller,Emil Mottola,Berndt Mueller,Benjamin Nachman,John Negele,John Orrell,Amol Patwardhan,Daniel Phillips,Stephen Poole,Irene Qualters,Mike Rumore,Thomas Schaefer,Jeremy Scott,Rajeev Singh,James Vary,Juan-Jose Galvez-Viruet,Kyle Wendt,Hongxi Xing,Liang Yang,Glenn Young,Fanyi Zhao
Journal
arXiv preprint arXiv:2303.00113
Published Date
2023/2/28
In preparation for the 2023 NSAC Long Range Plan (LRP), members of the Nuclear Science community gathered to discuss the current state of, and plans for further leveraging opportunities in, QIST in NP research at the Quantum Information Science for U.S. Nuclear Physics Long Range Planning workshop, held in Santa Fe, New Mexico on January 31 - February 1, 2023. The workshop included 45 in-person participants and 53 remote attendees. The outcome of the workshop identified strategic plans and requirements for the next 5-10 years to advance quantum sensing and quantum simulations within NP, and to develop a diverse quantum-ready workforce. The plans include resolutions endorsed by the participants to address the compelling scientific opportunities at the intersections of NP and QIST. These endorsements are aligned with similar affirmations by the LRP Computational Nuclear Physics and AI/ML Workshop, the Nuclear Structure, Reactions, and Astrophysics LRP Town Hall, and the Fundamental Symmetries, Neutrons, and Neutrinos LRP Town Hall communities.
Final Technical Report for" Search for Neutrinoless Double Beta Decay with EXO-200 and nEXO"
Authors
Douglas Beck,Liang Yang
Published Date
2023/9/22
The technical report summarizes the technical achievements of DOE award "Search for Neutrinoless Double Beta Decay with EXO-200 and nEXO" to the University of Illinois from 2018 - 2023.
LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
Authors
T Namikawa,AI Lonappan,C Baccigalupi,N Bartolo,D Beck,K Benabed,A Challinor,P Diego-Palazuelos,J Errard,S Farrens,A Gruppuso,N Krachmalnicoff,M Migliaccio,E Martínez-González,V Pettorino,G Piccirilli,M Ruiz-Granda,B Sherwin,J Starck,P Vielva,R Akizawa,A Anand,J Aumont,R Aurlien,S Azzoni,M Ballardini,AJ Banday,RB Barreiro,M Bersanelli,D Blinov,M Bortolami,T Brinckmann,E Calabrese,P Campeti,A Carones,F Carralot,FJ Casas,K Cheung,L Clermont,F Columbro,G Conenna,A Coppolecchia,F Cuttaia,G d'Alessandro,P de Bernardis,T de Haan,M De Petris,S Della Torre,E Di Giorgi,HK Eriksen,F Finelli,C Franceschet,U Fuskeland,G Galloni,M Galloway,M Georges,M Gerbino,M Gervasi,T Ghigna,S Giardiello,C Gimeno-Amo,E Gjerløw,M Hazumi,S Henrot-Versillé,LT Hergt,E Hivon,K Kohri,E Komatsu,L Lamagna,M Lattanzi,C Leloup,M Lembo,M López-Caniego,G Luzzi,B Maffei,S Masi,M Massa,S Matarrese,T Matsumura,S Micheli,A Moggi,M Monelli,L Montier,G Morgante,B Mot,L Mousset,R Nagata,P Natoli,A Novelli,I Obata,A Occhiuzzi,L Pagano,A Paiella,D Paoletti,G Pascual-Cisneros,V Pavlidou,F Piacentini,M Pinchera,G Pisano,G Polenta,G Puglisi,M Remazeilles,A Ritacco,A Rizzieri,J Rubino-Martin,Y Sakurai,D Scott,M Shiraishi,G Signorelli,SL Stever,Y Takase,H Tanimura,A Tartari,K Tassis,L Terenzi,M Tristram,L Vacher,B van Tent,IK Wehus,G Weymann-Despres,M Zannoni,Y Zhou
Journal
arXiv preprint arXiv:2312.05194
Published Date
2023/12/8
We estimate the efficiency of mitigating the lensing $B$-mode polarization, the so-called delensing, for the $LiteBIRD$ experiment with multiple external data sets of lensing-mass tracers. The current best bound on the tensor-to-scalar ratio, $r$, is limited by lensing rather than Galactic foregrounds. Delensing will be a critical step to improve sensitivity to $r$ as measurements of $r$ become more and more limited by lensing. In this paper, we extend the analysis of the recent $LiteBIRD$ forecast paper to include multiple mass tracers, i.e., the CMB lensing maps from $LiteBIRD$ and CMB-S4-like experiment, cosmic infrared background, and galaxy number density from $Euclid$- and LSST-like survey. We find that multi-tracer delensing will further improve the constraint on $r$ by about $20\%$. In $LiteBIRD$, the residual Galactic foregrounds also significantly contribute to uncertainties of the $B$-modes, and delensing becomes more important if the residual foregrounds are further reduced by an improved component separation method.
Search for MeV electron recoils from dark matter in EXO-200
Authors
S Al Kharusi,G Anton,I Badhrees,PS Barbeau,D Beck,V Belov,T Bhatta,M Breidenbach,T Brunner,GF Cao,WR Cen,C Chambers,B Cleveland,M Coon,A Craycraft,T Daniels,L Darroch,SJ Daugherty,J Davis,S Delaquis,A Der Mesrobian-Kabakian,R DeVoe,J Dilling,A Dolgolenko,MJ Dolinski,J Echevers,W Fairbank Jr,D Fairbank,J Farine,S Feyzbakhsh,P Fierlinger,YS Fu,D Fudenberg,P Gautam,R Gornea,G Gratta,C Hall,EV Hansen,J Hoessl,P Hufschmidt,M Hughes,A Iverson,A Jamil,C Jessiman,MJ Jewell,A Johnson,A Karelin,LJ Kaufman,T Koffas,R Krücken,A Kuchenkov,KS Kumar,Y Lan,A Larson,BG Lenardo,DS Leonard,GS Li,S Li,Z Li,C Licciardi,YH Lin,R MacLellan,T McElroy,T Michel,B Mong,DC Moore,K Murray,O Njoya,O Nusair,A Odian,I Ostrovskiy,A Perna,A Piepke,A Pocar,F Retière,AL Robinson,PC Rowson,D Ruddell,J Runge,S Schmidt,D Sinclair,K Skarpaas,AK Soma,V Stekhanov,M Tarka,S Thibado,M Todd,T Tolba,TI Totev,RHM Tsang,B Veenstra,V Veeraraghavan,P Vogel,J-L Vuilleumier,M Wagenpfeil,J Watkins,LJ Wen,U Wichoski,G Wrede,SX Wu,Q Xia,DR Yahne,L Yang,Y-R Yen,O Ya Zeldovich,T Ziegler,EXO-200 Collaboration
Journal
Physical Review D
Published Date
2023/1/30
We present a search for electron-recoil signatures from the charged-current absorption of fermionic dark matter using the EXO-200 detector. We report an average electron-recoil background rate of 6.8× 10 4 cts kg− 1 yr− 1 keV− 1 above 4 MeV and find no statistically significant excess over our background projection. Using a total Xe 136 exposure of 234.1 kg yr, we exclude new parameter space for the charged-current absorption cross section for dark matter masses between m χ= 2.6–11.6 MeV with a minimum of 6× 10− 51 cm 2 at 8.3 MeV at the 90% confidence level.
Sensitivity modeling for LiteBIRD
Authors
Takashi Hasebe,Peter AR Ade,A Adler,E Allys,D Alonso,K Arnold,D Auguste,Jonathan Aumont,R Aurlien,J Austermann,Susanna Azzoni,Carlo Baccigalupi,AJ Banday,R Banerji,RB Barreiro,N Bartolo,Susanta Basak,E Battistelli,Lucille Bautista,J Beall,D Beck,S Beckman,K Benabed,J Bermejo-Ballesteros,M Bersanelli,J Bonis,J Borrill,F Bouchet,F Boulanger,S Bounissou,Maksym Brilenkov,ML Brown,Martin Bucher,Erminia Calabrese,Marianina Calvo,P Campeti,A Carones,Francisco Javier Casas,A Catalano,A Challinor,V Chan,K Cheung,Y Chinone,J Cliche,F Columbro,W Coulton,Javier Cubas,A Cukierman,D Curtis,Giuseppe D’Alessandro,K Dachlythra,P de Bernardis,T de Haan,Elena de la Hoz,M De Petris,S Della Torre,C Dickinson,P Diego-Palazuelos,M Dobbs,T Dotani,D Douillet,Lionel Duband,Anne Ducout,S Duff,Jean-Marc Duval,Kako Ebisawa,T Elleflot,HK Eriksen,J Errard,T Essinger-Hileman,F Finelli,R Flauger,Cristian Franceschet,Unni Fuskeland,S Galli,M Galloway,K Ganga,JR Gao,RT Genova-Santos,M Gerbino,Massimo Gervasi,T Ghigna,Serena Giardiello,Ellen Gjerløw,Marcin Lukasz Gradziel,Julien Grain,Laurent Grandsire,Frank Grupp,A Gruppuso,JE Gudmundsson,NW Halverson,J Hamilton,P Hargrave,M Hasegawa,Makoto Hattori,M Hazumi,S Henrot-Versillé,LT Hergt,D Herman,D Herranz,CA Hill,G Hilton,E Hivon,RA Hlozek,Thuong D Hoang,AL Hornsby,Y Hoshino,J Hubmayr,K Ichiki,T Iida,H Imada,K Ishimura,H Ishino,G Jaehnig,M Jones,T Kaga,S Kashima,N Katayama,A Kato,T Kawasaki,Reijo Keskitalo,T Kisner,Y Kobayashi,N Kogiso,A Kogut,K Kohri,E Komatsu,K Komatsu,K Konishi,N Krachmalnicoff,I Kreykenbohm,CL Kuo,A Kushino,L Lamagna,JV Lanen,G Laquaniello,M Lattanzi,AT Lee,C Leloup,F Levrier,E Linder,T Louis,Gemma Luzzi,J Macias-Perez,T Maciaszek,B Maffei,D Maino,M Maki,S Mandelli,M Maris
Journal
Journal of Low Temperature Physics
Published Date
2023/6
LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three telescopes with transition-edge sensor bolometers. In this work we estimated the LiteBIRD instrumental sensitivity using its current design. We estimated the detector noise due to the optical loadings using physical optics and ray-tracing simulations. The noise terms associated with thermal carrier and readout noise were modeled in the detector noise calculation. We calculated the observational sensitivities over fifteen bands designed for the LiteBIRD telescopes using assumed observation time efficiency.
Fundamental neutron physics: a white paper on progress and prospects in the US
Authors
R Alarcon,A Aleksandrova,S Baeßler,DH Beck,T Bhattacharya,M Blatnik,TJ Bowles,JD Bowman,J Brewington,LJ Broussard,A Bryant,JF Burdine,J Caylor,Y Chen,JH Choi,L Christie,TE Chupp,V Cianciolo,V Cirigliano,SM Clayton,B Collett,C Crawford,W Dekens,M Demarteau,D DeMille,G Dodson,BW Filippone,N Floyd,N Fomin,J Fry,K Fuyuto,S Gardner,R Godri,R Golub,F Gonzalez,GL Greene,V Gudkov,R Gupta,J Hamblen,L Hayen,J C Hendrus,K Hickerson,FB Hills,AT Holley,S Hoogerheide,M Hubert,PR Huffman,SK Imam,TM Ito,L Jin,G Jones,A Komives,E Korobkina,W Korsch,KKH Leung,C-Y Liu,K-F Liu,JC Long,D Mathews,A Mendelsohn,E Mereghetti,P Mohanmurthy,CL Morris,P Mueller,HP Mumm,A Nelsen,A Nicholson,J Nico,CM O'Shaughnessy,PA Palamure,S Pastore,RW Pattie Jr,NS Phan,JA Pioquinto,B Plaster,D Počanić,H Rahangdale,R Redwine,A Reid,DJ Salvat,A Saunders,D Schaper,C-Y Seng,M Singh,A Shindler,WM Snow,Z Tang,A Walker-Loud,DK-T Wong,F Wietfeldt,AR Young
Published Date
2023/8/17
Fundamental neutron physics, combining precision measurements and theory, probes particle physics at short range with reach well beyond the highest energies probed by the LHC. Significant US efforts are underway that will probe BSM CP violation with orders of magnitude more sensitivity, provide new data on the Cabibbo anomaly, more precisely measure the neutron lifetime and decay, and explore hadronic parity violation. World-leading results from the US Fundamental Neutron Physics community since the last Long Range Plan, include the world's most precise measurement of the neutron lifetime from UCN, the final results on the beta-asymmetry from UCNA and new results on hadronic parity violation from the NPDGamma and n-He runs at the FNPB (Fundamental Neutron Physics Beamline), precision measurement of the radiative neutron decay mode and n-He at NIST. US leadership and discovery potential are ensured by the development of new high-impact experiments including BL3, Nab, LANL nEDM and nEDM@SNS. On the theory side, the last few years have seen results for the neutron EDM from the QCD term, a factor of two reduction in the uncertainty for inner radiative corrections in beta-decay which impacts CKM unitarity, and progress on {\it ab initio} calculations of nuclear structure for medium-mass and heavy nuclei which can eventually improve the connection between nuclear and nucleon EDMs. In order to maintain this exciting program and capitalize on past investments while also pursuing new ideas and building US leadership in new areas, the Fundamental Neutron Physics community has identified a …
BICEP Array: 150 GHz detector module development
Authors
Alessandro Schillaci,PAR Ade,Z Ahmed,M Amiri,D Barkats,R Basu Thakur,CA Bischoff,D Beck,JJ Bock,V Buza,J Cheshire,J Connors,J Cornelison,Mike Crumrine,A Cukierman,E Denison,M Dierickx,L Duband,M Eiben,S Fatigoni,JP Filippini,C Giannakopoulos,N Goeckner-Wald,D Goldfinger,JA Grayson,P Grimes,G Hall,G Halal,M Halpern,E Hand,S Harrison,S Henderson,SR Hildebrandt,GC Hilton,J Hubmayr,H Hui,KD Irwin,J Kang,KS Karkare,S Kefeli,JM Kovac,CL Kuo,Kenny Lau,EM Leitch,A Lennox,KG Megerian,OY Miller,L Minutolo,L Moncelsi,Y Nakato,T Namikawa,HT Nguyen,R O’Brient,S Palladino,M Petroff,Nathan Precup,T Prouve,C Pryke,B Racine,CD Reintsema,BL Schmitt,B Singari,A Soliman,T St Germaine,B Steinbach,RV Sudiwala,KL Thompson,C Tucker,AD Turner,C Umiltà,C Verges,AG Vieregg,A Wandui,AC Weber,DV Wiebe,J Willmert,WLK Wu,E Yang,KW Yoon,E Young,C Yu,L Zeng,C Zhang,S Zhang
Journal
Journal of Low Temperature Physics
Published Date
2023/12
The Background Imaging of Cosmic Extragalactic Polarization (BICEP)/Keck (BK) collaboration is currently leading the quest for the highest-sensitivity measurements of the polarized cosmic microwave background (CMB) anisotropies on a degree scale with a series of cryogenic telescopes, of which BICEP Array (BA) is the latest Stage-3 upgrade with a total of 32,000 detectors. The instrument comprises 4 receivers spanning 30–270 GHz, with the low-frequency 30/40 GHz deployed to the South Pole Station in late 2019. The full complement of receivers is forecast to set the most stringent constraints on the tensor-to-scalar ratio r. Building on these advances, the overarching small-aperture telescope concept is already being used as the reference for further Stage-4 experiment design. This paper describes the development of the BICEP Array 150 GHz detector module and its fabrication requirements, with …
Search for two-neutrino double-beta decay of Xe to the excited state of Ba with the complete EXO-200 dataset
Authors
S Al Kharusi,G Anton,I Badhrees,PS Barbeau,D Beck,V Belov,T Bhatta,M Breidenbach,T Brunner,GF Cao
Journal
Chin. Phys. C
Published Date
2023
A new search for two-neutrino double-beta (2νββ) decay of Xe to the excited state of Ba is performed with the full EXO-200 dataset. A deep learning-based convolutional neural network is used to discriminate signal from background events. Signal detection efficiency is increased relative to previous searches by EXO-200 by more than a factor of two. With the addition of the Phase II dataset taken with an upgraded detector, the median 90% confidence level half-life sensitivity of 2νββ decay to the state of Ba is yr using a total Xe exposure of 234.1 kg yr. No statistically significant evidence for 2νββ decay to the state is observed, leading to a lower limit of yr at 90% confidence level, improved by 70% relative to the current world's best constraint.
BICEP/Keck. XVII. Line-of-sight distortion analysis: estimates of gravitational lensing, anisotropic cosmic birefringence, patchy reionization, and systematic errors
Authors
PAR Ade,Z Ahmed,M Amiri,D Barkats,R Basu Thakur,CA Bischoff,D Beck,JJ Bock,H Boenish,E Bullock,V Buza,JR Cheshire IV,J Connors,J Cornelison,M Crumrine,A Cukierman,EV Denison,M Dierickx,L Duband,M Eiben,S Fatigoni,JP Filippini,S Fliescher,C Giannakopoulos,N Goeckner-Wald,DC Goldfinger,J Grayson,P Grimes,G Hall,G Halal,M Halpern,E Hand,S Harrison,S Henderson,SR Hildebrandt,J Hubmayr,H Hui,KD Irwin,J Kang,KS Karkare,E Karpel,S Kefeli,SA Kernasovskiy,JM Kovac,CL Kuo,K Lau,EM Leitch,A Lennox,KG Megerian,L Minutolo,L Moncelsi,Y Nakato,T Namikawa,HT Nguyen,R O’Brient,RW Ogburn IV,S Palladino,M Petroff,T Prouve,C Pryke,B Racine,CD Reintsema,S Richter,A Schillaci,R Schwarz,BL Schmitt,CD Sheehy,B Singari,A Soliman,T St Germaine,B Steinbach,RV Sudiwala,GP Teply,KL Thompson,JE Tolan,C Tucker,AD Turner,C Umiltà,C Vergès,AG Vieregg,A Wandui,AC Weber,DV Wiebe,J Willmert,CL Wong,WLK Wu,H Yang,KW Yoon,E Young,C Yu,L Zeng,C Zhang,S Zhang,BICEP/Keck Collaboration
Journal
The Astrophysical Journal
Published Date
2023/5/25
We present estimates of line-of-sight distortion fields derived from the 95 and 150 GHz data taken by BICEP2, BICEP3, and the Keck Array up to the 2018 observing season, leading to cosmological constraints and a study of instrumental and astrophysical systematics. Cosmological constraints are derived from three of the distortion fields concerning gravitational lensing from large-scale structure, polarization rotation from magnetic fields or an axion-like field, and the screening effect of patchy reionization. We measure an amplitude of the lensing power spectrum . We constrain polarization rotation, expressed as the coupling constant of a Chern–Simons electromagnetic term g aγ≤ 2.6× 10− 2/H I, where H I is the inflationary Hubble parameter, and an amplitude of primordial magnetic fields smoothed over 1 Mpc B 1Mpc≤ 6.6 nG at 95 GHz. We constrain the rms of optical depth fluctuations in a simple" …
D. H. Beck FAQs
What is D. H. Beck's h-index at University of Illinois at Urbana-Champaign?
The h-index of D. H. Beck has been 142 since 2020 and 195 in total.
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The articles with the titles of
1: 2 AV CONDUCTION LEADING TO INAPPROPRIATE ICD SHOCK
NSR Query Results
Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
A Natural Field-like Entanglement Resource in Trapped-Ion Chains
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers
Entanglement structures in quantum field theories. II. Distortions of vacuum correlations through the lens of local observers
BICEP/Keck. XVI. Characterizing dust polarization through correlations with neutral hydrogen
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are the top articles of D. H. Beck at University of Illinois at Urbana-Champaign.
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